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Resonant stripping as the origin of dwarf spheroidal galaxies

Author

Listed:
  • Elena D'Onghia

    (Institute for Theoretical Physics, University of Zurich
    Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 51, Cambridge, Massachusetts 02138, USA)

  • Gurtina Besla

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 51, Cambridge, Massachusetts 02138, USA)

  • Thomas J. Cox

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 51, Cambridge, Massachusetts 02138, USA)

  • Lars Hernquist

    (Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 51, Cambridge, Massachusetts 02138, USA)

Abstract

Galaxies stripped for action A new theory for the formation of dwarf spheroidal galaxies identifies encounters between dwarf disk galaxies and somewhat larger dwarfs as the likely source. Dwarf spheroids are dark-matter-dominated low luminosity galaxies in the nearby Universe and their origin is one of the outstanding puzzles of how galaxies form. Previous models are relevant only to dwarf spheroidals orbiting close to a giant galaxy like the Milky Way or Andromeda, and are ruled out as general theories because of the existence of dwarfs in the outskirts of the Local Group. In the new model simulations, encounters between dwarf galaxies in small groups excite a 'resonant stripping' process that transforms them into dwarf spheroidals before they are accreted by systems like the Milky Way. Within this framework, dwarf spheroidals should form and interact in pairs or small groups, leaving detectable long stellar streams and tails.

Suggested Citation

  • Elena D'Onghia & Gurtina Besla & Thomas J. Cox & Lars Hernquist, 2009. "Resonant stripping as the origin of dwarf spheroidal galaxies," Nature, Nature, vol. 460(7255), pages 605-607, July.
  • Handle: RePEc:nat:nature:v:460:y:2009:i:7255:d:10.1038_nature08215
    DOI: 10.1038/nature08215
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